Effects of Light-Emitting Diode (LED) Red and Blue Light on the Growth and Photosynthetic Characteristics of <i>Momordica charantia</i>L.

With andromonoecious Momordica charantia L. (bitter gourd) as material, three light qualities (50 μmol·m-2·s-1) including white LED light (WL), blue monochromatic light (B, 465 nm), and red monochromatic light (R, 650 nm) were carried out to investigate their effects on seed germination, physiological and biochemical parameters, sex differentiation and photosynthetic characteristics of bitter gourd. The results showed that compared to the WL treatment, the R treatment significantly promoted seed germination, seedling height elongation and soluble sugar content, the B treatment significantly increased seedling stem diameter, reducing sugar content and soluble protein content, the R and B treatments both significantly reduced sucrose content, but their POD activity showed no significant difference. Compared with the R treatment, the B treatment significantly increased the total female flower number and female flower nod ratio in 30 nods of main stems. The study of photosynthetic characteristics found that the R and B treatments could effectively increase the stomatal conductance (GS) of leaves, significantly improved the net photosynthetic rate (Pn) compared to the WL treatment, and the effect of the B treatment was better. Compared to the R and WL treatments, the B treatment increased the maximum photosynthetic rate (Pmax), apparent quantum efficiency (AQE) and light saturation point (LSP), and reduced the dark respiration rate (Rd) and light compensation point (LCP) of the leaves. Fit light response curves showed that the adaptability and utilization of weak light in bitter gourd were middle or below, but it showed higher adaptability and utilization of strong light. Thus, it suggests that Momordica charantia is a typical sun plan with lower Rd. In summary, it is concluded that blue light has a positive effect on the seed germination, seedling growth, sex differentiation and improving the photosynthetic performance, and this will lay the foundation for artificially regulating optimum photosynthesis using specific LEDs wavelength, and help to elucidate the relationship how light quality influences the sex differentiation of plant.

众包物流平台建设中的服务模式创新研究

众包物流是传统物流发展到一定阶段而产生的适合经济社会发展及物流业服务创新的一种重要物流服务方式。与传统物流方式不同,众包物流的参与人员不局限于专业的物流业者,而是广泛吸纳了社会大众,使得物流有了新的发展内涵。本文通过分析传统物流发现其有一些局限性。在此基础上,结合近年来出现的物流新业态——众包物流探讨了众包物流的应用及现状,指出了众包物流的应用难点和痛点,也列明了众包物流的诸多优势,同时讨论了构建众包物流服务模式创新平台的具体方式和途径。

On delay-dependent robust stability of neutral systems

The delay-dependent robust stability of uncertain linear neutral systems with delays is investigated. Both discrete-delay-dependent/neutral-delay-independent and neutral-/discrete- delay-dependent stability criteria will be developed. The proposed stability criteria are formulated in the form of linear matrix inequalities and it is easy to check the robust stability of the considered systems. By introducing certain Lyapunov-Krasovskii functional the mathematical development of our result avoids model transformation and bounding for cross terms, which lead to conservatism. Finally, numerical example is given to indicate the improvement over some existing results.

基于STM-32的红外语音控制系统

目的:设计一种低成本、适应性强的基于WIFI的智能家居网关的语音控制系统。方法:搭建基于STM-32单片机内核的硬件平台,通过语音指令的收集处理和识别,做出相应反馈,并通过WIFI和红外射频做媒介,达到远程控制家电的目的。结果:经实验测试表明,文章所设计的智能家居网关能够很好的满足智能家居控制系统对家居环境智能化的需求。结论:以STM-32为核心的智能家居网关系统的方案可行,为廉价智能家居的推广提供了参考依据。

Contention-Based Beaconless Real-Time Routing Protocol for Wireless Sensor Networks

This paper presents a novel real-time routing protocol, called CBRR, with less energy consumption for wireless sensor networks (WSNs). End-to-End real-time requirements are fulfilled with speed or delay constraint at each hop through integrating the contention and neighbor table mechanisms. More precisely, CBRR maintains a neighbor table via the contention mechanism being dependent on wireless broadcast instead of beacons. Comprehensive simulations show that CBRR can not only achieve higher performance in static networks, but also work well for dynamic networks.

JUNO sensitivity on proton decay p→νK^(+)searches

The Jiangmen Underground Neutrino Observatory(JUNO)is a large liquid scintillator detector designed to explore many topics in fundamental physics.In this study,the potential of searching for proton decay in the p→νK^(+)mode with JUNO is investigated.The kaon and its decay particles feature a clear three-fold coincidence signature that results in a high efficiency for identification.Moreover,the excellent energy resolution of JUNO permits suppression of the sizable background caused by other delayed signals.Based on these advantages,the detection efficiency for the proton decay via p→νK^(+)is 36.9%±4.9%with a background level of 0.2±0.05(syst)±0.2(stat)events after 10 years of data collection.The estimated sensitivity based on 200 kton-years of exposure is 9.6×1033 years,which is competitive with the current best limits on the proton lifetime in this channel and complements the use of different detection technologies.

川西地区雷口坡组四段天然气成藏特征及勘探前景

中三叠统雷口坡组是四川盆地西部近年来海相天然气勘探的热点层系之一,业内对其成藏条件和气藏类型的认识存在较大分歧。研究表明,川西地区雷口坡组四段油气成藏条件优越,潮坪相白云岩储层大规模稳定展布,二叠系和中三叠统雷口坡组2套烃源岩发育。雷四段在川西坳陷由西向东发育3种成藏模式,即跨层烃源断裂+裂缝复合输导的下生上储式构造气藏,小型烃源断裂+层内裂缝“接力式”输导的下生上储式构造—地层气藏,以及层内裂缝输导的自生自储式岩性气藏。除了目前已获得超千亿方探明储量的川西龙门山前雷四段构造气藏外,坳陷东侧雷口坡组四段尖灭线附近为探索构造—地层气藏的有利区域,坳陷东侧斜坡带中下部(广汉斜坡带)是探索岩性气藏的有利区域。

优化多色激光场产生单个阿秒脉冲的理论模拟

多色组合激光场是一种产生超短孤立阿秒脉冲的可能选通方案.以800 nm飞秒激光作为基频场,利用遗传算法优化双色和三色激光场参数,根据超快光场相干合成技术得到了亚周期激光场.利用优化激光脉冲驱动氖原子即可产生超连续高次谐波并获得单个阿秒脉冲.在考虑宏观传播效应并采取合理参数(激光强度、气体压强、气体靶长度和位置)的情况下,利用球形空间滤波器选择合理空间范围的谐波,得到了中心能量约为200 eV、脉宽约为50 as的单个阿秒脉冲.理论模拟中充分考虑了目前的激光技术和实验条件,本研究结果可为实验室产生超短阿秒脉冲提供重要的理论指导.

Feasibility and physics potential of detecting ^(8)B solar neutrinos at JUNO

The Jiangmen Underground Neutrino Observatory(JUNO)features a 20 kt multi-purpose underground liquid scintillator sphere as its main detector.Some of JUNO's features make it an excellent location for^8B solar neutrino measurements,such as its low-energy threshold,high energy resolution compared with water Cherenkov detectors,and much larger target mass compared with previous liquid scintillator detectors.In this paper,we present a comprehensive assessment of JUNO's potential for detecting^8B solar neutrinos via the neutrino-electron elastic scattering process.A reduced 2 MeV threshold for the recoil electron energy is found to be achievable,assuming that the intrinsic radioactive background^(238)U and^(232)Th in the liquid scintillator can be controlled to 10^(-17)g/g.With ten years of data acquisition,approximately 60,000 signal and 30,000 background events are expected.This large sample will enable an examination of the distortion of the recoil electron spectrum that is dominated by the neutrino flavor transformation in the dense solar matter,which will shed new light on the inconsistency between the measured electron spectra and the predictions of the standard three-flavor neutrino oscillation framework.IfDelta m^(2)_(21)=4.8times10^(-5);(7.5times10^(-5))eV^(2),JUNO can provide evidence of neutrino oscillation in the Earth at approximately the 3sigma(2sigma)level by measuring the non-zero signal rate variation with respect to the solar zenith angle.Moreover,JUNO can simultaneously measureDelta m^2_(21)using^8B solar neutrinos to a precision of 20% or better,depending on the central value,and to sub-percent precision using reactor antineutrinos.A comparison of these two measurements from the same detector will help understand the current mild inconsistency between the value of Delta m^2_(21)reported by solar neutrino experiments and the KamLAND experiment.

Sub-percent precision measurement of neutrino oscillation parameters with JUNO

JUNO is a multi-purpose neutrino observatory under construction in the south of China.This publication presents new sensitivity estimates for the measurement of the △m_(31)^(2),△m_(21)^(2),sin^(2)θ_(12),and sin^(2)θ_(13) oscillation parameters using reactor antineutrinos,which is one of the primary physics goals of the experiment.The sensitivities are obtained using the best knowledge available to date on the location and overburden of the experimental site,the nuclear reactors in the surrounding area and beyond,the detector response uncertainties,and the reactor antineutrino spectral shape constraints expected from the TAO satellite detector.It is found that the △m_(21)^(2) and sin^(2)θ_(12) oscillation parameters will be determined to 0.5%precision or better in six years of data collection.In the same period,the △m_(31)^(2) parameter will be determined to about 0.2%precision for each mass ordering hypothesis.The new precision represents approximately an order of magnitude improvement over existing constraints for these three parameters.